Skip to main content
Cornell University
We gratefully acknowledge support from the Simons Foundation, member institutions, and all contributors. Donate
arxiv logo > astro-ph > arXiv:2103.01968

Help | Advanced Search

arXiv logo
Cornell University Logo

quick links

  • Login
  • Help Pages
  • About

Astrophysics > High Energy Astrophysical Phenomena

arXiv:2103.01968 (astro-ph)
[Submitted on 2 Mar 2021 (v1), last revised 14 Oct 2021 (this version, v3)]

Title:Real-time Discovery of AT2020xnd: A Fast, Luminous Ultraviolet Transient with Minimal Radioactive Ejecta

Authors:Daniel A. Perley (LJMU), Anna Y. Q. Ho (Berkeley), Yuhan Yao (Caltech), Christoffer Fremling (Caltech), Joseph P. Anderson (ESO), Steve Schulze (Stockholm), Harsh Kumar (IIT Bombay), G. C. Anupama (IIA), Sudhanshu Barway (IIA), Eric C. Bellm (UW), Varun Bhalerao (IIT Bombay), Ting-Wan Chen (Stockholm), Dmitry A. Duev (Caltech), Lluís Galbany (UAB), Matthew J. Graham (Caltech), Mariusz Gromadzki (Warsaw), Claudia P. Gutiérrez (FINCA/Tuorla), Nada Ihanec (Warsaw), Cosimo Inserram (Cardiff), Mansi M. Kasliwal (Caltech), Erik C. Kool (Stockholm), S. R. Kulkarni (Caltech), Russ R. Laher (IPAC), Frank J. Masci (IPAC), James D. Neill (Caltech), Matt Nicholl (Birmingham), Miika Pursiainen (DTU), Joannes van Roestel (Caltech), Yashvi Sharma (Caltech), Jesper Sollerman (Stockholm), Richard Walters (Caltech), Philip Wiseman (Southampton)
View a PDF of the paper titled Real-time Discovery of AT2020xnd: A Fast, Luminous Ultraviolet Transient with Minimal Radioactive Ejecta, by Daniel A. Perley (LJMU) and 31 other authors
View PDF
Abstract:The many unusual properties of the enigmatic AT2018cow suggested that at least some subset of the empirical class of fast blue optical transients (FBOTs) represents a genuinely new astrophysical phenomenon. Unfortunately, the intrinsic rarity and fleeting nature of these events have made it difficult to identify additional examples early enough to acquire the observations necessary to constrain theoretical models. We present here the Zwicky Transient Facility discovery of AT2020xnd (ZTF20acigmel, the "Camel") at z=0.243, the first unambiguous AT2018cow analog to be found and confirmed in real time. AT2018cow and AT2020xnd share all key observational properties: a fast optical rise, sustained high photospheric temperature, absence of a second peak attributable to ejection of a radioactively-heated stellar envelope, extremely luminous radio, millimetre, and X-ray emission, and a dwarf-galaxy host. This supports the argument that AT2018cow-like events represent a distinct phenomenon from slower-evolving radio-quiet supernovae, likely requiring a different progenitor or a different central engine. The sample properties of the four known members of this class to date disfavour tidal disruption models but are consistent with the alternative model of an accretion powered jet following the direct collapse of a massive star to a black hole. Contextual filtering of alert streams combined with rapid photometric verification using multi-band imaging provides an efficient way to identify future members of this class, even at high redshift.
Comments: Accepted to MNRAS
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE)
Cite as: arXiv:2103.01968 [astro-ph.HE]
  (or arXiv:2103.01968v3 [astro-ph.HE] for this version)
  https://doi.org/10.48550/arXiv.2103.01968
arXiv-issued DOI via DataCite
Related DOI: https://doi.org/10.1093/mnras/stab2785
DOI(s) linking to related resources

Submission history

From: Daniel Perley [view email]
[v1] Tue, 2 Mar 2021 19:00:01 UTC (1,098 KB)
[v2] Fri, 20 Aug 2021 22:03:53 UTC (1,100 KB)
[v3] Thu, 14 Oct 2021 15:19:10 UTC (1,100 KB)
Full-text links:

Access Paper:

    View a PDF of the paper titled Real-time Discovery of AT2020xnd: A Fast, Luminous Ultraviolet Transient with Minimal Radioactive Ejecta, by Daniel A. Perley (LJMU) and 31 other authors
  • View PDF
  • TeX Source
  • Other Formats
view license
Ancillary-file links:

Ancillary files (details):

  • photometry.txt
Current browse context:
astro-ph.HE
< prev   |   next >
new | recent | 2021-03
Change to browse by:
astro-ph

References & Citations

  • INSPIRE HEP
  • NASA ADS
  • Google Scholar
  • Semantic Scholar

1 blog link

(what is this?)
a export BibTeX citation Loading...

BibTeX formatted citation

×
Data provided by:

Bookmark

BibSonomy logo Reddit logo

Bibliographic and Citation Tools

Bibliographic Explorer (What is the Explorer?)
Connected Papers (What is Connected Papers?)
Litmaps (What is Litmaps?)
scite Smart Citations (What are Smart Citations?)

Code, Data and Media Associated with this Article

alphaXiv (What is alphaXiv?)
CatalyzeX Code Finder for Papers (What is CatalyzeX?)
DagsHub (What is DagsHub?)
Gotit.pub (What is GotitPub?)
Hugging Face (What is Huggingface?)
Papers with Code (What is Papers with Code?)
ScienceCast (What is ScienceCast?)

Demos

Replicate (What is Replicate?)
Hugging Face Spaces (What is Spaces?)
TXYZ.AI (What is TXYZ.AI?)

Recommenders and Search Tools

Influence Flower (What are Influence Flowers?)
CORE Recommender (What is CORE?)
IArxiv Recommender (What is IArxiv?)
  • Author
  • Venue
  • Institution
  • Topic

arXivLabs: experimental projects with community collaborators

arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website.

Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them.

Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs.

Which authors of this paper are endorsers? | Disable MathJax (What is MathJax?)
  • About
  • Help
  • contact arXivClick here to contact arXiv Contact
  • subscribe to arXiv mailingsClick here to subscribe Subscribe
  • Copyright
  • Privacy Policy
  • Web Accessibility Assistance
  • arXiv Operational Status
    Get status notifications via email or slack